File:Galaxis Scheibe Umlaufsperiode.png

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Deutsch: Umlaufsperioden für die epizyklische Bewegung eines Sterns in der galaktischen Scheibe in Abh. vom Abstand von der Rotationsachse auf Grundlage der Dichteverteilung nach McMillan, Mass models of the Milky Way, in: Monthly Notices of the Royal Astronomical Society 414 S.2466ff, 2011 sowie des stellardynamischen Modells von Oort J.H., Stellar Dynamic, in: Stars and Stellar Systems Band 5, Kap.21, S.455 ff, 1965. Die blaue Kurve zeigt die Umlaufsperiode des Epizykels um das galaktische Zentrum, die rote die Umlaufsperiode des Sterns um den Epizykel. Es wird ein reines Scheibenmodell ohne Berücksichtigung der Linse (Bulge) und des Halo betrachtet.
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Author Michael Oestreicher

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Date/TimeThumbnailDimensionsUserComment
current16:41, 25 October 2015Thumbnail for version as of 16:41, 25 October 20151,889 × 1,417 (103 KB)Michael Oestreicher (talk | contribs)More recent modell for galactic disc used (see corrected description of diagram)
16:44, 22 September 2015Thumbnail for version as of 16:44, 22 September 20151,889 × 1,417 (97 KB)Michael Oestreicher (talk | contribs)User created page with UploadWizard

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